Observation of the peculiar OH maser G24.3+0.1

Details Observation of the peculiar OH maser G24.3+0.1 Observation of the peculiar OH maser G24.3+0.1

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..726p&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Oct. 1984, p. 726-729) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Sept.-Oc

Astronomy and Astrophysics

Astronomy

Hydroxyl Emission, Interstellar Masers, Radio Sources (Astronomy), Linear Polarization, Radial Velocity, Stellar Evolution, Superhigh Frequencies

Scientific paper

18 cm OH observations and accurate position measurements of the peculiar maser source G24.3+0.1 were carried out. The profile of the 1667 MHz OH line consists of many variable emission features in the large velocity range from +60 to +120 km/s. An OH emission source of the type IIc has been detected near the maser. The G24.3+0.1 source seems to be a type Ia circumstellar maser in a star-formation region.

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